activity
20152020
most citedFinite-frequency sensitivity kernels in spherical geometry for time-distance helioseismology

13 citations · 20 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20202 cited

A general formulation for computing spherical helioseismic sensitivity kernels while incorporating systematical effects

Jishnu Bhattacharya, Shravan M. Hanasoge, Katepalli R. Sreenivasan

As helioseismology matures and turns into a precision science, modeling finite-frequency, geometric and systematical effects is becoming increasingly important. Here we introduce a…

astro-ph.SR2019

Validating time-distance helioseismic inversions for non-separable subsurface profiles of an average supergranule

Vedant Dhruv, Jishnu Bhattacharya, Shravan Hanasoge

Supergranules are divergent 30-Mm sized cellular flows observed everywhere at the solar photosphere. Their place in the hierarchy of convective structures and their origin remain p…

astro-ph.SR20175 cited

Iterative inversion of synthetic travel times successful at recovering sub-surface profiles of supergranular flows

Jishnu Bhattacharya, Shravan M. Hanasoge, Aaron C. Birch +1

We develop a helioseismic inversion algorithm that can be used to recover sub-surface vertical profiles of 2-dimensional supergranular flows from surface measurements of synthetic…

astro-ph.SR201713 cited

Finite-frequency sensitivity kernels in spherical geometry for time-distance helioseismology

Krishnendu Mandal, Jishnu Bhattacharya, Samrat Halder +1

The inference of internal properties of the Sun from surface measurements of wave travel times is the goal of time-distance helioseismology. A critical step toward the accurate int…

astro-ph.SR2015

Frequency shifts of resonant modes of the Sun due to near-surface convective scattering

Jishnu Bhattacharya, Shravan. M. Hanasoge, H. M. Antia

Measurements of oscillation frequencies of the Sun and stars can provide important independent constraints on their internal structure and dynamics. Seismic models of these oscilla…